Brittle strength of basaltic rock masses with applications to Venus

Details Brittle strength of basaltic rock masses with applications to Venus Brittle strength of basaltic rock masses with applications to Venus

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9810883s&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. E6, p. 10,883-10,895.

Physics

29

Basalt, Fracture Strength, Planetary Composition, Planetary Mass, Rock Mechanics, Venus Surface, Lava, Modulus Of Elasticity, Poisson Ratio, Satellite Observation, Venus, Strength, Basalt, Terrestrial Planets, Lava Flow, Parameters, Compression, Fracturing, Laboratory Studies, Experiments, Temperature, Thermal Effects, Deformation, Depth, Extension, Subsurface, Stress, Elasticity, Faulting

Scientific paper

Spacecraft images of surfaces with known or suspected basaltic composition on Venus (as well as on moon and Mars) indicate that these rocks have been deformed in the brittle regime to form faults and perhaps joints, in addition to folding and more distributed types of deformation. This paper presents results of detailed examinations and interpretations of Venus surface materials which show that the strengths of basaltic rocks on planetary surfaces and in the shallow subsurface are significantly different from strength values commonly used in tectonic modeling studies which assume properties of either intact rock samples or single planar shear surface.

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